Galaxy Models with Third Integrals

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Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..259b&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Mathematics

Logic

15

Scientific paper

Kinematic and morphological data for our Galaxy require models that take full account of a third integral. This paper concentrates on third integrals which are actions. These enjoy important advantages over other third integrals and can be calculated for most numerically-integrated orbits by spectral techniques. The structure of the halo and disk of the Galaxy is explored in the space (J-space) of these actions.

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